ALMA and VLA observations of the outflows in IRAS 16293-2422

被引:32
作者
Loinard, Laurent [1 ,2 ]
Zapata, Luis A. [1 ]
Rodriguez, Luis F. [1 ]
Pech, Gerardo [1 ]
Chandler, Claire J. [3 ]
Brogan, Crystal L. [4 ]
Wilner, David J. [5 ]
Ho, Paul T. P. [5 ,6 ]
Parise, Berengere [2 ]
Hartmann, Lee W. [7 ]
Zhu, Zhaohuan [8 ]
Takahashi, Satoko [6 ]
Trejo, Alfonso [6 ]
机构
[1] Univ Nacl Autonoma Mexico, Ctr Radiostron & Astrofis, Morelia 58089, Michoacan, Mexico
[2] Max Planck Inst Radioastron, D-53121 Bonn, Germany
[3] Natl Radio Astron Observ, Socorro, NM 87801 USA
[4] Natl Radio Astron Observ, Charlottesville, VA 22903 USA
[5] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[6] Acad Sinica, Inst Astron & Astrophys, Taipei 115, Taiwan
[7] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA
[8] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
关键词
techniques: interferometric; stars: formation; stars: individual: IRAS 16293-2422; ISM: jets and outflows; 1ST HYDROSTATIC CORE; SOLAR-TYPE PROTOSTAR; SUBMILLIMETER ARRAY; MULTIPLE SYSTEM; PROPER MOTIONS; STAR-FORMATION; RADIO-SOURCES; IRAS-16293-2422; INFALL; OPHIUCHUS;
D O I
10.1093/mnrasl/sls038
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present Atacama Large Millimeter/submillimeter Array (ALMA) and Very Large Array (VLA) observations of the molecular and ionized gas at 0.1-0.3 arcsec resolution in the Class 0 protostellar system IRAS 16293-2422. These data clarify the origins of the protostellar outflows from the deeply embedded sources in this complex region. Source A2 is confirmed to be at the origin of the well-known large-scale north-east-south-west flow. The most recent VLA observations reveal a new ejection from that protostar, demonstrating that it drives an episodic jet. The central compact part of the other known large-scale flow in the system, oriented roughly east-west, is well delineated by the CO(6-5) emission imaged with ALMA and is confirmed to be driven from within component A. Finally, a one-sided blueshifted bubble-like outflow structure is detected here for the first time from source B to the northwest of the system. Its very short dynamical time-scale (similar to 200 yr), low velocity and moderate collimation support the idea that source B is the youngest object in the system, and possibly one of the youngest protostars known.
引用
收藏
页码:L10 / L14
页数:5
相关论文
共 32 条
[1]  
Arce H. G., 2007, Protostars and Planets V, P245, DOI 10.48550/arXiv.astro-ph/0603071
[2]  
BODENHEIMER P, 1995, ANNU REV ASTRON ASTR, V33, P199
[3]   A multiple system of radio sources at the core of the L723 multipolar outflow [J].
Carrasco-Gonzalez, Carlos ;
Anglada, Guillem ;
Rodriguez, Luis F. ;
Torrelles, Jose M. ;
Osorio, Mayra ;
Girart, Jose M. .
ASTROPHYSICAL JOURNAL, 2008, 676 (02) :1073-1081
[4]   Multiple shocks around the low-luminosity protostar IRAS 16293-2422 [J].
Castets, A ;
Ceccarelli, C ;
Loinard, L ;
Caux, E ;
Lefloch, B .
ASTRONOMY & ASTROPHYSICS, 2001, 375 (01) :40-53
[5]  
Ceccarelli C, 2000, ASTRON ASTROPHYS, V355, P1129
[6]   IRAS 16293-2422: Proper motions, jet precession, the hot core, and the unambiguous detection of infall [J].
Chandler, CJ ;
Brogan, CL ;
Shirley, YL ;
Loinard, L .
ASTROPHYSICAL JOURNAL, 2005, 632 (01) :371-396
[7]   L1448 IRS2E: A CANDIDATE FIRST HYDROSTATIC CORE [J].
Chen, Xuepeng ;
Arce, Hector G. ;
Zhang, Qizhou ;
Bourke, Tyler L. ;
Launhardt, Ralf ;
Schmalzl, Markus ;
Henning, Thomas .
ASTROPHYSICAL JOURNAL, 2010, 715 (02) :1344-1351
[8]   The solar type protostar IRAS16293-2422: new constraints on the physical structure [J].
Crimier, N. ;
Ceccarelli, C. ;
Maret, S. ;
Bottinelli, S. ;
Caux, E. ;
Kahane, C. ;
Lis, D. C. ;
Olofsson, J. .
ASTRONOMY & ASTROPHYSICS, 2010, 519
[9]   DETECTION OF A BIPOLAR MOLECULAR OUTFLOW DRIVEN BY A CANDIDATE FIRST HYDROSTATIC CORE [J].
Dunham, Michael M. ;
Chen, Xuepeng ;
Arce, Hector G. ;
Bourke, Tyler L. ;
Schnee, Scott ;
Enoch, Melissa L. .
ASTROPHYSICAL JOURNAL, 2011, 742 (01)
[10]   A CANDIDATE DETECTION OF THE FIRST HYDROSTATIC CORE [J].
Enoch, Melissa L. ;
Lee, Jeong-Eun ;
Harvey, Paul ;
Dunham, Michael M. ;
Schnee, Scott .
ASTROPHYSICAL JOURNAL LETTERS, 2010, 722 (01) :L33-L38